japanese vlbi activities and east asian vlbi network

Japanese VLBI activities and East Asian VLBI Network

H.Kobayashi(NAOJ)November,23,2011

2011South African SKA, Postgraduate Bursary Conference

March,11,2011Earthquakes

Antenna were damaged at Mizusawa and Ibaraki .

Mizusawa

Ibaraki

Tokyo

M9

Fukushima

Ibaraki station has two 32-m telescopes, which were used as Intelsat stations

March 11th Earthquake 　 effects

Mizusawa(VERA) ; Collision of Elevation gear and housing

Ibaraki station damages

Displacement of Mizusawa

~3m 　 displacement of the station

2500

km

5000 km

East Asian VLBI Network

Current working VLBI stations in Eastern Asia is 20 !

Japan(13)• VERA(4), Kashima, Tsukuba, Yamaguchi,

Nobeyama, Usuda, Tomakomai, 　 Gifu, 　Uchinoura, Takahagi, Hitachi

Korea(3)• KVN (3) Yonsei, Ulsan, Tamna

China(4)• Shanghai, Urumqi, Beijin, Kumming• Shanghai 65m 　 under construction

East Asia VLBI consortium

(under East Asia Core Observatory Association)

2004~

Japanese VLBI network

VERA

Korean VLBI network Chinese VLBI network

Total effective aperture and baseline length

VLBI array EAVN VLBA EVN

No. of Stations

２０ １０ １２

Baseline length

5,000km 8,000km 2,000km-8,000km

Effective Aperture @8GHz

9,000m2 3,700m2 9,800m2

Effective Aperture @22GHz

4,900m2 3,200m2 4,900m2

Effective 　Aperture @43GHz

1,400m2 2,900m2 1,800m2

UV-coverage by EAVN

Declination +30 deg. 0 deg. -30 deg.

Observation features Phase referencing observations

• VERA 2 beam• KVN multi-frequency• Nodding -> high sensitivity observations for low Tb objects

(RQQ, SNR, Galactic objects) ->astrometry for maser sources (H2O,SiO,CH3OH..)

High dynamic range observations• 8GHz and 22GHz mainly• 86GHz and 129 GHz with 4(+1) stations

Seoul VLBI correlator center

Opened on May 13th, 2010

8Gbps x 16 station Largest VLBI correlator

New Seoul correlator for KVN/EAVN

Mark5BKVN/CVN

DIR-2000VERA

K-5JVN

Optical Fiber

VLBIData

Buffer(VDB2000)

CorrelationSubsystem

8Gbps 16 stations

DataArchive

Correlator Control & Operation S/W

From 2012, operation will be started !

OCTAVE(8Gbps Disc recorder)

1 or 2 Gbps× ４I/O

VSI-H － 10 GbEConverterOCTAVIA 10 GbE

10 GbEHub

10 GbE

Disk ServerOCTDISK

VSI-H

Disk Server

Disk Server

Disk Server

２

2Gbps x 4

Ethernet transmission

Science (Dec. 5,2008)

EAVN observtaions

KVN/VERA : Some scientific verification observations are on going.• 22GHz/43GHz mapping• Geodesy• 43GHz SgrA* etc.

CVN(Shanghai)/JVN • Methanol(C band) observations• X band mapping test ?

Ibaraki, Shanghai, VERAx4○Observations・ Date 　　 Aug. 28 and 29 ,2010 ○Results　　 Methanol maser maps of 22 sources　　 Jet/Disk structure and velocity field

Schedule 2010-2011 　　

• Test Observations with VERA+KVN, JVN+CVN

2011-2012• Start of science observations with Japan

(VERA,JVN) +Korea (KVN), and Japan(JVN)+China(CVN).

2013• Start of science observations with Japan,

Korea and China

Simultaneous Multi-Frequency Obs. -Phase Compensation, mm-VLBI

Constructions of three stations were completed on Dec. 2008 !

Freq. Band S Band X Band K Band Q Band Freq. Range 2.2 ~ 2.8 GHz 8 ~ 9 GHz 21.5 ~23.5 GHz 42 ~ 44 GHz

Rx Noise < 25 K < 25 K < 30 K < 50 K 1st IF / BW 2.5G/600MHz 8.5G/1GHz 8.5G/2GHz 8.5G/2GHz IF Power -20 dBm -20 dBm -20 dBm -20 dBm

Polarization LCP/RCP LCP/RCP LCP/RCP LCP/RCP

* 86, 129 GHz Receivers will be installed.

Prototype 43 GHz Re-ceiver

Receiver

Major Facilities for RA in China

Delingha 13.7m

21CMA

L,C,S/X,K

S/X

L,C(5/6G),S/X,K

S/X

L,C,S/X:2012Ku,K,Ka:Q:2015

L,C:2012K :?

Yellow:plan L,C,X:2014

VLBI in China

ITS-CSCC2008 22

FAST (Five hundred meter Aperture Spherical radio Telescope)

Taiwan Project of Submillimeter VLBI

• ALMA prototype antenna (12m, ～３０ μ ｒｍｓ） will be moved to Greenland.

• 230/350 GHz VLBI ALMA, SMA, LMT, CARMA ・・・・・

Japanese VLBI Network (JVN) Collaboration

• NAOJ (VERA)• Hokkaido, Ibaraki, Tsukuba,

Gifu, Osaka-Pref, Yamaguchi, Kagoshima university

• JAXA, NICT, GSI• 13 telescopes (11m ~ 64m)

Purpose• A new, characteristic VLBI

array• A Base of East-Asian VLBI

Progress• Started in 2004• Steady Observation in 2005• First Paper published in 2006

Observing time ~200 hr/yr

• EAVN test observation

26

Our Milky way galaxy map by VERA

Ｓ２６９ １５０００l.y.

Orion Nebula １４００l.y.

First phase variations between 2 beams

Honma, et al, 2003 PASJ 55

Fringe phase of W49N,OH43 and difference Allan variance of them

Scientific goal Astrometry with 10μarcsec. accuracy

between background object and galactic object within 2.2 degree separation• Proper motion and parallax measurements

3D map and velocity field of the Galaxy Detailed 3D velocity structure of molecular gas

around evolved stars and star forming regions

VERA scientific goal Measurements of

distance and proper motions of galactic maser objects (H2O,SiO)

Dynamics of the Galaxy Maser object:

　　 luminous point-like objects

-> triangulation point of the Galaxy !

Current status of astrometry with VERA

Ro = 8.35±0.44 　 kpc

Rotation Curve of Galaxy

KDDI(telecom) passed on Intelsat stations to NAOJ

Yamaguchi 32m Ibaraki 32mx2

Cooled C&X band and K band RXs are equipped.

2500

km

5000 km

East Asian VLBI Network

Conclusion East Asian VLBI Network is organizing with

Japan, Korea and China. EAVN is comparable array to VLBA and

EVN. It has good features for phase referencing and astrometry.

From 2012, science array observation with Japan, Korea, and China is expected.

VERA has carried out astrometry observations with precise phase referencing VLBI.